The Small Satellites of Pluto as Observed by New Horizons

H. A. Weaver , M. W. Buie , B. J. Buratti , W. M. Grundy , T. R. Lauer , C. B. Olkin , A. H. Parker , S. B. Porter

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M. R. Showalter J. R. Spencer S. A. Stern A. J. Verbiscer W. B. McKinnon J. M. Moore S. J. Robbins P. Schenk K. N. Singer O. S. Barnouin A. F. Cheng C. M. Ernst C. M. Lisse D. E. Jennings A. W. Lunsford D. C. Reuter D. P. Hamilton D. E. Kaufmann K. Ennico L. A. Young R. A. Beyer R. P. Binzel V. J. Bray A. L. Chaikin J. C. Cook D. P. Cruikshank C. M. Dalle Ore A. M. Earle G. R. Gladstone C. J. A. Howett I. R. Linscott F. Nimmo J. Wm. Parker S. Philippe S. Protopapa H. J. Reitsema B. Schmitt T. Stryk M. E. Summers C. C. C. Tsang H. H. B. Throop O. L. White A. M. Zangari

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classification 🌌 astro-ph.EP

keywords moonssmallapproxhydraplutofourhorizonskerberos

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The New Horizons mission has provided resolved measurements of Pluto's moons Styx, Nix, Kerberos, and Hydra. All four are small, with equivalent spherical diameters of $\approx$40 km for Nix and Hydra and ~10 km for Styx and Kerberos. They are also highly elongated, with maximum to minimum axis ratios of $\approx$2. All four moons have high albedos ( $\approx$50-90 %) suggestive of a water-ice surface composition. Crater densities on Nix and Hydra imply surface ages $\gtrsim$ 4 Ga. The small moons rotate much faster than synchronous, with rotational poles clustered nearly orthogonal to the common pole directions of Pluto and Charon. These results reinforce the hypothesis that the small moons formed in the aftermath of a collision that produced the Pluto-Charon binary.

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The Small Satellites of Pluto as Observed by New Horizons

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